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Astronomical units of length
From Wikipedia, the free encyclopedia
Astronomers use a number of different length units for different objects. The length unit used is typically determined by two criteria:
- the unit should create manageable numbers
- the unit should be easily derivable from observation
The distances are closely related to the cosmic distance ladder.
| Astronomical Range | Typical Units |
|---|---|
| Distances to satellites | kilometres |
| Planetary distances | astronomical units |
| Distances to nearby stars | parsecs, light years |
| Distances at the galactic scale | kiloparsecs |
| Distances to nearby galaxies | megaparsecs |
The distances to distant galaxies are typically not quoted in distance units at all, but rather in terms of redshift. The reasons for this are that converting redshift to distance requires knowledge of the Hubble constant which was not accurately measured until the early 21st century, and that at cosmological distances, the curvature of space-time allows one to come up with multiple definitions for distance. For example, the distance as defined by the amount of time it takes for a light beam to travel to you is different from the distance as defined by the apparent size of an object.